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Table 1.

Properties of the lines detected towards the molecular arc in CrA.

Transitions ν(a) Eup (a) log10(Aul) (a) gu (a) δVchan (a) ncr (c) I [K km s−1] (a)
(MHz) (K) (s−1) (km s−1) (104 cm−3) “A” “B” “C”
CH3OH-A (80, 8-71, 7) 95 169.391 84 −5.37 68 1.54 1.3–1.4 8.6 4.1 6.1
CH3OH-A (21, 2-11, 1) 95 914.310 22 −5.60 20 1.54 2.0–2.1 4.1 1.8 3.9
CH3OH-A (31, 3-40, 4) 107 013.831 28 −5.51 28 0.17 3.2–3.5 4.5 < 2.6 2.8
SiO (5-4) 217 104.980 31 −3.28 11 0.51 153.1–156.1 1.2 3.7 < 0.6
CH3OH-E (42, 3-31, 2) 218 440.063 46 −4.33 36 0.17 24.3–23.4 19.2 8.6 9.2
p-H2CO (30, 3-20, 2) 218 222.192 21 −3.55 7 0.17 160.1–183.0 14.3 8.9 17.9
CH3OH-A (51, 4-41, 3) 243 915.788 50 −4.22 44 0.15 19.9–21.1 6.9 3.9

Notes. (a)Spectroscopic data from The Cologne Database for Molecular Spectroscopy (Müller et al. 2005). (b)The SiO (5-4) spectrum is smoothed in velocity by a factor of three to increase sensitivity. (c)Critical densities obtained considering downward collision rates in a multilevel system and a temperature range of 50–100 K (Sect. 3.3). Collisional rates taken from the LAMDA database (Schöier et al. 2005), based on Balança et al. (2018) for SiO, Wiesenfeld & Faure (2013) for p-H2CO and Rabli & Flower (2010) for the A- and E-type CH3OH. (d)We assume an uncertainty of 20%. Regions “A”, “B”, and “C” are centred at the peak positions of CH3OH (42, 3–31, 2), SiO (5–4), and p-H2CO (30, 3–20, 2), respectively (see Fig. 2).

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